A dataset provided by the European Space Agency

Name 069366
Title Unveiling the most massive clusters at z>0.5 with Planck and XMM-Newton.
URL

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DOI 10.5270/esa-ngf0ztw
Author Dr monique arnaud
Description We propose to gather spatially resolved spectroscopy of a sample of 33 massive (M_{500}>5e+14 solar masses) clusters detected blindly by Planck and confirmed to-day to be in the redshift range 0.5
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Discovery of radio haloes and double relics in distant MACS galaxy clusters: clues to the efficiency of particle acceleration . Bonafede, A., Bruggen, M., et all. . MNRAS . 426-40 . 2012 . 2012MNRAS.426...40B ,
Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO . Mroczkowski, T., Kovacs, A., et all. . ApJ . 808-6 . 2015 . 2015ApJ...808L...6M ,
New XMM-Newton observation of the Phoenix cluster: properties of the cool core . Tozzi, P., Gastaldello, F., et all. . A&A . 580-6 . 2015 . 2015A&A...580A...6T ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71 . Ruppin, F., Adam, R., et all. . A&A . 597-110 . 2017 . 2017A&A...597A.110R ,
Pr...
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2012-05-19T04:12:10Z/2013-01-13T18:44:14Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2014-02-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-02-05T00:00:00Z, 069366, 17.56_20190403_1200. https://doi.org/10.5270/esa-ngf0ztw